dc.contributor.author | Kostensalo, Joel | |
dc.contributor.author | Suhonen, Jouni | |
dc.contributor.author | Zuber, K. | |
dc.date.accessioned | 2020-03-10T12:51:45Z | |
dc.date.available | 2020-03-10T12:51:45Z | |
dc.date.issued | 2020 | |
dc.identifier.citation | Kostensalo, J., Suhonen, J., & Zuber, K. (2020). Calculated solar-neutrino capture rate for a radiochemical 205Tl-based solar-neutrino detector. <i>Physical Review C</i>, <i>101</i>(3), Article 031302(R). <a href="https://doi.org/10.1103/PhysRevC.101.031302" target="_blank">https://doi.org/10.1103/PhysRevC.101.031302</a> | |
dc.identifier.other | CONVID_34932685 | |
dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/68117 | |
dc.description.abstract | Radiochemical experiments for low-energy solar-neutrino detection have been making headlines by exploiting
the isotopes 37Cl and 71Ga. Such a very low-threshold measurement of this type can also be performed using 205Tl, which has been considered for decades for this purpose. A unique feature of this detector nucleus is the
integration in the solar-neutrino flux over 106 of years owing to its long-living daughter 205Pb. In this Rapid
Communication, we have calculated for the first time the cross section for the charged-current solar-neutrino
scattering off 205Tl. Taking into account the solar-model-predicted neutrino fluxes and the electron-neutrino
survival probabilities, a solar-neutrino capture rate of 62.2 ± 8.6 solar-neutrio units is determined, a value
significantly smaller than in previous estimates. | en |
dc.format.mimetype | application/pdf | |
dc.language | eng | |
dc.language.iso | eng | |
dc.publisher | American Physical Society | |
dc.relation.ispartofseries | Physical Review C | |
dc.rights | In Copyright | |
dc.subject.other | electroweak interactions in nuclear physics | |
dc.subject.other | nuclear structure and decays | |
dc.subject.other | nucleus-neutrino interactions | |
dc.subject.other | solar neutrinos | |
dc.title | Calculated solar-neutrino capture rate for a radiochemical 205Tl-based solar-neutrino detector | |
dc.type | research article | |
dc.identifier.urn | URN:NBN:fi:jyu-202003102355 | |
dc.contributor.laitos | Fysiikan laitos | fi |
dc.contributor.laitos | Department of Physics | en |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
dc.description.reviewstatus | peerReviewed | |
dc.relation.issn | 2469-9985 | |
dc.relation.numberinseries | 3 | |
dc.relation.volume | 101 | |
dc.type.version | publishedVersion | |
dc.rights.copyright | ©2020 American Physical Society | |
dc.rights.accesslevel | openAccess | fi |
dc.type.publication | article | |
dc.relation.grantnumber | 318043 | |
dc.subject.yso | ydinfysiikka | |
dc.subject.yso | hiukkasfysiikka | |
dc.subject.yso | neutriinot | |
dc.format.content | fulltext | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p14759 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p15576 | |
jyx.subject.uri | http://www.yso.fi/onto/yso/p5219 | |
dc.rights.url | http://rightsstatements.org/page/InC/1.0/?language=en | |
dc.relation.doi | 10.1103/PhysRevC.101.031302 | |
dc.relation.funder | Research Council of Finland | en |
dc.relation.funder | Suomen Akatemia | fi |
jyx.fundingprogram | Academy Project, AoF | en |
jyx.fundingprogram | Akatemiahanke, SA | fi |
jyx.fundinginformation | This work has been partially supported by the Academy of Finland under Academy Project No. 318043. J.K. acknowledges financial support from the Jenny and Antti Wihuri Foundation. | |
dc.type.okm | A1 | |